4.1 Article

Sr-Nd-Pb isotopic constraints on the nature of the mantle sources involved in the genesis of the high-Ti tholeiites from northern Parana Continental Flood Basalts (Brazil)

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PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.jsames.2013.04.004

关键词

Parana Continental Flood Basalts; Mantle sources; High-TiO2 basalts; Sr-Nd-Pb isotopic systematics; Mantle plume

资金

  1. FAPESP
  2. CNPq
  3. CAPES (PNPD program)

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There has been little research on geochemistry and isotopic compositions in tholeiites of the Northern region from the Parana Continental Flood Basalts (PCFB), one of the largest continental provinces of the world. In order to examine the mantle sources involved in the high-Ti (Pitanga and Paranapanema) basalt genesis, we studied Sr, Nd, and Pb isotopic systematics, and major, minor and incompatible trace element abundances. The REE patterns of the investigated samples (Pitanga and Paranapanema magma type) are similar (parallel to) to those of Island Arc Basalts' REE patterns. The high-Ti basalts investigated in this study have initial (133 Ma) Sr-87/Sr-86 ratios of 0.70538-0.70642, Nd-143/Nd-144 of 0.51233-0.51218, Pb-206/Pb-204 of 17.74-18.25, Pb-207/Pb-204 of 15.51-15.57, and Pb-208/Pb-204 of 38.18-38.45. These isotopic compositions do not display any correlation with Nb/Th, Nb/La or P2O5/K2O ratios, which also reflect that these rocks were not significantly affected by low-pressure crustal contamination. The incompatible trace element ratios and Sr Nd Pb isotopic compositions of the PCFB tholeiites are different to those found in Tristan da Cunha ocean island rocks, showing that this plume did not play a substantial role in the PCFB genesis. This interpretation is corroborated by previously published osmium isotopic data (initial gamma(Os) values range from +1.0 to +2.0 for high-Ti basalts), which also preclude basalt generation by melting of ancient subcontinental lithospheric mantle. The geochemical composition of the northern PCFB may be explained through the involvement of fluids and/or small volume melts related to metasomatic processes. In this context, we propose that the source of these magmas is a mixture of sublithospheric peridotite veined and/or interlayered with mafic components (e.g., pyroxenites or eclogites). The sublithospheric mantle (dominating the osmium isotopic compositions) was very probably enriched by fluids and/or magmas related to the Neoproterozoic subduction processes. This sublithospheric mantle region may have been frozen and coupled to the base of the Parana basin lithospheric plate above which the Paleozoic subsidence and subsequent Early Cretaceous magmatism occurred. (C) 2013 Elsevier Ltd. All rights reserved.

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